共查询到20条相似文献,搜索用时 78 毫秒
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用射频磁控溅射技术在蓝宝石衬底上制备了一组不同衬底温度的Mn掺杂ZnO薄膜。质子激发X射线荧光(PIXE)测量表明,薄膜中仅有含量为5 at.%的Mn,未见其它磁性杂质元素(如Fe、Co、Ni等)。同步辐射X射线衍射(SR-XRD)表明,这些Mn掺杂ZnO薄膜具有纤锌矿ZnO结构。SR-XRD和扩展X射线吸收精细结构谱(EXAFS)分析显示,薄膜中未发现Mn团簇或MnO、MnO2、Mn2O3、Mn3O4等二次相,Mn原子是通过替代Zn原子而进入了ZnO晶格。 相似文献
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Y2-xSmxW3012(x=0.0~0.4)样品通过传统固相反应合成,用X射线粉末衍射测定了样品的晶体结构。室温X射线粉末衍射在中国科学院研究生院无机材料实验室的MSAL-XD2X射线粉末衍射仪上进行, 相似文献
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采用X射线衍射和正电子湮没多普勒展宽测量相结合,研究了纳米晶态材料Fe73.5Cu1Nb3Si13.5B9的结构随退火温度的变化。实验结果表明:急冷非品样品在480℃开始明显晶化,基体中析出体心立方结构的α-Fe(Si)固溶体。随着退火温度的升高,非晶漫射峰不断减弱,而晶态相的衍射谱逐渐增强。进一步计算对衍射谱的分离,给出了品化分数和非晶相平均原子间距随退火温度的变化规律。正电子湮没实验证实了约550℃退火时样品内出现以Nb、B原子为主的晶界非晶相,S参数随退火温度的变化与非晶相平均原子间距随退火温度的变化规律一致。 相似文献
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利用金刚石压砧高压装置(DAC),对Ca3Mn2O7的粉末样品进行了高压能散X射线衍射实验。结果表明,由于岩盐层易被压缩,在压力作用下层状钙钛矿结构锰氧化物Ca3Mn2O7的结构不稳定。在0-35GPa压力范围内,Ca3Mo2O7晶体结构发生了两次相变。在1.3GPa左右,由原来的四方相变为正交相,在9.5GPa左右,又由正交相向新的四方相转变。 相似文献
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Fe73.5Cu1Nb3Si13.5B9非晶合金化过程的X射线衍射和正电子湮没研究 总被引:1,自引:0,他引:1
采用X射线衍射和正电子湮没多普勒展宽测量相结合,研究了纳米晶态材料Fe73.5Cu1Nb3Si13.5B9的结构随退火温度的变化。实验结果表明:急冷非晶样品在480℃开始明显晶化,基体中析出体心立方结构的α-Fe(Si)固溶体。随着退火温度的高,非晶漫峰不断减弱,而晶态相的衍射谱逐渐增强。进一步计算对衍射谱的分离,给出了晶化分数和非晶相平均原子间距随退火温度的变化规律。正电子湮没实验证实了约550 相似文献
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利用X射线粉末衍射仪和超导量子干涉磁强计(SQUID)对RxEr5-xSi3(R=Nd,Dy)系列化合物的晶体结构、相组成及磁性能进行了研究,探讨了替代原子种类和含量对其结构和性能的影响。 相似文献
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利用电弧炉制备了DyxEr5-xSi3(x=0,1,2,3,4,5)系列化合物样品。通过X射线粉末衍射分析和磁性测量研究了Dy替代Er对Er5Si3化合物晶体结构和磁性的影响。结果表明:DyxEr5-xSi3(x=0,1,2,3,4,5)系列化合物的晶体结构为Mn5Si3型,随着Dy替代量的增加,晶胞体积变大。当0≤x≤2时,样品具有反铁磁性,顺磁居里温度由负值(x=0)变为正值;而x=3,4时,样品显现铁磁性,顺磁居里温度均为正值。虽然磁性原子及其相互作用的变化对磁性能影响很大,但所有样品的磁有序转变温度都很好地遵守了DeGennes定律。 相似文献
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本文对电缆X射线辐照响应的机理和模拟方法进行了研究,分析了电缆直流和脉冲X射线辐照响应的异同。建立了带状电缆X射线辐照响应一维计算模型,该模型包含电缆屏蔽层和介质层间隙、介质层瞬态辐射感应电导率等计算模型,模拟了带状电缆直流和脉冲X射线辐照电流响应。模拟结果表明,在X射线注量相同的条件下,电缆直流和方波脉冲X射线响应具有类似的波形特征及相同的间隙电压。因此,在该计算模型描述的电缆X射线辐照响应机制下,可利用直流X射线开展相应的脉冲X射线辐照响应机制模拟。 相似文献
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凸度检测系统中X光机参数对厚度测量精度的影响 总被引:2,自引:2,他引:0
X射线凸度检测技术可在线获得板带材的断面轮廓并反馈到连轧系统实现实时凸度控制,在冶金工业中得到广泛应用,是冶金自动化中的关键技术。该项技术存在厚度测量范围大、测量精度要求高的特点。本文通过理论分析厚度测量精度与X光机管电压和管电流的关系,得到X光机管电流是决定系统极限测量精度的主要因素,X光机管电压是决定系统测量厚度范围的主要因素。在此基础上给出了由测量精度确定管电流的方法和由测量范围确定管电压的方法,为系统X光机的选型和测量档位设定提供指导依据。 相似文献
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Yan A Wu X 《Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms》2011,269(16):1841-1843
In the inline phase contrast X-ray tomography the reconstructed apparent linear attenuation coefficient values may be greatly larger than sample’s linear attenuation coefficients or even be negative. In this work we present a general formula to quantitatively relate the apparent linear attenuation coefficient values in cone-beam phase contrast tomography to sample’s linear attenuation coefficients and refractive indices. This formula overcomes the gross inaccuracy of the existing formula in the literature in analyzing high-resolution phase contrast tomography, and it will be useful for correctly interpreting and quantifying the apparent linear attenuation coefficients in cone-beam X-ray phase contrast tomography. 相似文献
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E.S. Valamontes J.C. Statharas C. Nomicos 《Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms》2007,260(2):628-632
In this paper, we used back-foil scanning X-ray microfluorescence (SXRF) and we examined the sensitivity of the technique for the analysis of very thin overlayers, where electron probe X-ray microanalysis (EPMA) reaches its detection limits. The lateral resolution of back-foil SXRF is also calculated for all the systems used. Both experimental results and Monte-Carlo calculations are used in this respect. Back-foil SXRF used in optimized experimental conditions, is found to be more sensitive than EPMA, especially in the case of very thin overlayers. The lateral resolution of back-foil SXRF is of the order of some micrometers. This is much better than the lateral resolution in conventional XRF and of the same order of magnitude as in EPMA. 相似文献
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使用X光聚束系统的X射线荧光分析研究 总被引:2,自引:0,他引:2
复合光导管组成的X光透镜可将发散的X光束聚至直径φ0.5mm,聚束后的功率密度增加10^4倍,这种新型的X光透镜已用于X射线荧光分析研究,使用X光管功率仅2W,而探测限可达10^-9-10^10g. 相似文献
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Keisuke TanizawaTetsuo Sekiya Shigeo OhshioHiroki Akasaka Hidetoshi Saitoh 《Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms》2011,269(3):313-317
The development of an intense X-ray source using backscattered X-ray produced using an advanced electrode configuration is described. The electrodes were composed of field emitters deposited on a wire mounted on a perforated plate as the cathode and a copper plate as the anode. Electrons from these emitters collided with the copper plate and X-ray was generated at collision points. The backscattered X-ray in the direction normal to the electron trajectory through a hole in the anode escaped from the vacuum chamber through a beryllium window. Continuous and characteristic X-rays were detected at an applied voltage lower than that of a conventional X-ray source from 3.0 to 9.4 kV, respectively. Moreover, the X-ray dosage measured with a survey meter reached 0.95 mSv/h at 5.0 kV of applied voltage. The transmission images of three types of material used as an X-ray source for the X-ray imaging system indicate three advantages; low power consumption, focal point controllable by adjusting applied voltage, and photographable motion picture of X-ray transmission. 相似文献
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Sunil Kumar Nirmal Singh 《Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms》2010,268(15):2437-2445
A tabulation of characteristic X-ray energies across the periodic table are provided where those X-rays are expected to result in a significant fractional resonant Raman scattering (RRS) contribution to the X-ray attenuation from a particular shell/subshell of the same or another element. The tabulations can be considered as guideline so as to know what can be expected due to RRS in typical photon- and particle-induced X-ray emission spectrometry. The RRS contribution is not included in the available theoretical attenuation coefficients, which are generally used in estimation of the matrix corrections in routine quantitative elemental analysis based on various X-ray emission techniques. The radiative RRS peaks can also interfere with normal X-ray spectrum and influence the elemental analysis. The RRS cross-section depends upon the energy difference of the X-ray energy and the shell/subshell ionization threshold taken in the units of the shell/subshell energy width, density of available states near the Fermi level, and the band structure in case the element is in the solid form. Some aspects of the dependence of the RRS contribution on the chemical forms of the elements are also discussed. 相似文献